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The quantum yield of a radiation-induced process is the number of times that a defined event occurs per photon absorbed by the system. Thus, the quantum yield is a measure of the efficiency with which absorbed light produces some effect.

For example, in a chemical photodegradation process, when a molecule falls apart after absorbing a light quantum, the quantum yield is the number of destroyed molecules divided by the number of photons absorbed by the system. Since not all photons are absorbed productively, the typical quantum yield will be less than 1.

Quantum yields greater than 1 are possible for photo-induced or radiation-induced chain reactions, in which a single photon may trigger a long chain of transformations. One example is the reaction of hydrogen with chlorine, in which a few hundred molecules of hydrochloric acid are typically formed per quantum of blue light absorbed.

In optical spectroscopy, the quantum yield is the probability that a given quantum state is formed from the system initially prepared in some other quantum state. For example, a singlet to triplet transition quantum yield is the fraction of molecules that, after being photoexcited into a singlet state, cross over to the triplet state. The fluorescence quantum yield is defined as the ratio of the number of photons emitted to the number of photons absorbed.

Experimentally, relative fluorescence quantum yields can be determined by measuring fluorescence of a fluorophore of known quantum yield with the same experimental parameters (excitation wavelength, slit widths, photomultiplier voltage etc.) as the substance in question. The quantum yield is then calculated by:

where Φ is the quantum yield, Int is the area under the emission peak (on a wavelength scale), A is absorbance at the excitation wavelength, and n is the refractive index of the sample. The subscript R denotes the respective values of the reference substance.

An improved determination is done by measuring the emission intensities over a range of optical densities, usually with and using the slope of the resulting line instead. In this case, the equation becomes:

where is the slope of the integrated fluorescence intensity with respect to the absorbance at the excitation wavelength of the sample and the subscript samp (as in ) denotes the values corresponding to the sample to be determined.

A more detailed description of this can be found at the link below listed in the external links section from Jobin Yvon.

See also

Quantum Efficiency Quantum yield can be defined by the equation: Q= photons emitted/photons absorbed. Quantum yield is essentially the emission efficiency of a given fluorochrome.

External links

• Recording Fluorescence Quantum Yields

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• This page was last modified on 3 November 2008, at 06:48.

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